Spectral energy distribution of TOI-4862. Red symbols represent the observed photometric measurements, and the horizontal bars represent the effective width of the passband. Blue symbols are the model fluxes from the best-fit PHOENIX atmosphere model (black). The absolute flux-calibrated Gaia spectrum is shown as a grey swathe in the inset figure. We note that the discrepancy between the blue points and PHOENIX atmosphere model at the shortest wavelengths is due to the SED being so steep in the UV that the nominal band-pass effective wavelength ends up being different from the flux-weighted effective wavelength.